The initial conditions of isolated star formation - VII. Spitzer mapping of pre-stellar cores

Details The initial conditions of isolated star formation - VII. Spitzer mapping of pre-stellar cores The initial conditions of isolated star formation - VII. Spitzer mapping of pre-stellar cores

2006-11-06

arxiv.org/abs/astro-ph/0611165v1

Mon.Not.Roy.Astron.Soc.375:843-854,2007

Astronomy and Astrophysics

Astrophysics

13 pages, 6 figures, accepted for publication by MNRAS

Scientific paper

10.1111/j.1365-2966.2006.11250.x

We have retrieved Spitzer archive data of pre-stellar cores taken with the Multiband Imaging Photometer for Spitzer (MIPS) at a wavelength of 160 um. Seventeen images, containing eighteen cores, were constructed. Flux densities were measured for each core, and background estimates were made. Mean off-source backgrounds were found to be 48\pm10 MJy/sr in Taurus and 140\pm55 MJy/sr in Ophiuchus. Consistency was found between the MIPS 170um and ISOPHOT 160um calibration. Fourteen cores were detected both by MIPS and our previous submillimetre surveys. Spectral Energy Distributions (SEDs) were made for each core, using additional 24- and 70-um data from the Spitzer data archive, as well as previous infra-red and submillimetre data. Previous temperature estimates were refined, and new temperature estimates were made where no Infrared Space Observatory (ISO) data exist. A temperature range of 8-18K was found for the cores, with most lying in the range 10-13K. We discount recent claims that a large number of pre-stellar cores may have been misclassified and in fact contain low luminosity protostars detectable only by Spitzer. We find no new protostars in our sample other than that previously reported in L1521F. It is shown that this has a negligible effect on pre-stellar lifetime estimates.

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